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Table 2

Literature values compared to our adopted effective temperature, surface gravity, and metallicity.

HD 209458
Teff [K] log g [cm s-2] [Fe/H] Reference Method

6000 4.25 0.00 Mazeh et al. (2000) spectroscopic
6063 4.38 0.04 Gonzalez et al. (2001) spectroscopic
6080 4.33 −0.06 Mashonkina & Gehren (2001) spectroscopic
5987 4.24 −0.04 Sadakane et al. (2002) spectroscopic
6100 4.50 −0.02 Heiter & Luck (2003) spectroscopic
6117 4.48 0.02 Santos et al. (2004) spectroscopic
5993 Ramírez & Meléndez (2004) photometric
6099 4.38 0.02 Valenti & Fischer (2005) spectroscopic
6118 4.50 0.03 Sousa et al. (2008) spectroscopic
4.368 Southworth (2009) light curve
6108 4.33 −0.04 Casagrande et al. (2011) photometric

6095 4.3 0.00 adopted (3D model) spectroscopic
6000 4.3 0.00 adopted (1D model) spectroscopic

HD 189733
Teff [K] log g [cm s-2] [Fe/H] Reference Method

5050 4.53 −0.03 Bouchy et al. (2005) spectroscopic
4939 van Belle & von Braun (2009) photometric
4.610 Southworth (2010) light curve
5022 4.58 −0.13 Casagrande et al. (2011) photometric

5050 4.53 0.00 adopted (3D model) spectroscopic
5000 4.53 0.00 adopted (1D model) spectroscopic

Notes. Quoted metallicities could not be corrected for differences in the assumed solar composition, as the latter was not always specified in the cited publications, leading to artificial offsets in [Fe/H].

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